A Possible Explanation of W-type Phenomena in V694 Peg
Three sets of complete multicolor light curves of V694 Peg observed in 2013, 2015, and 2019 were presented and analyzed. Our photometric solutions show that this system was an A-type shallow contact binary in 2013 and 2015 while it converted to a W-type ...
Hu-Shan Xu, Li-Ying Zhu
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Eclipsing binaries in local group galaxies: Physical properties of the stars and calibration of the zero-point of the cosmic distance scale [PDF]
E. F. Guinan +2 more
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Interferometric observations of the circumstellar disk environments in close binary stars
F. Eupen
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HEARTBEAT STARS: SPECTROSCOPIC ORBITAL SOLUTIONS FOR SIX ECCENTRIC BINARY SYSTEMS [PDF]
Rachel Smullen, Henry A. Kobulnicky
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Properties of Wolf-Rayet binaries: the key to understanding Wolf-Rayet stars [PDF]
A. F. J. Moffat
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ellc: A fast, flexible light curve model for detached eclipsing binary stars and transiting exoplanets [PDF]
P. F. L. Maxted
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Formation of twin compact stars in low-mass X-ray binaries [PDF]
S. Chanlaridis +7 more
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Two New Close Binary Central Stars of Planetary Nebulae from a Critically Selected Southern Hemisphere Sample [PDF]
T. C. Hillwig
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